! Started logfile: /vlbi/vcs9/uvm//J2259-3548_C_a_dfm.log on Tue Dec 26 23:13:32 2017 float field_size field_size = 1024 float field_cell field_cell = 0.3000 float taper_size taper_size = 40.0 float freq freq = 4.12800 obs /vlbi/vcs9/uvm//J2259-3548_C_a_uvm.fits ! Reading UV FITS file: /vlbi/vcs9/uvm//J2259-3548_C_a_uvm.fits ! AN table 1: 92 integrations on 21 of 21 possible baselines. ! AN table 2: 89 integrations on 1 of 1 possible baselines. ! AN table 3: 92 integrations on 1 of 1 possible baselines. ! Apparent sampling: 0.895409 visibilities/baseline/integration-bin. ! Found source: J2259-3548 ! ! There are 8 IFs, and a total of 8 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 4.128e+09 3.2e+07 1 3.2e+07 ! 02 2 4.16e+09 3.2e+07 1 3.2e+07 ! 03 3 4.192e+09 3.2e+07 1 3.2e+07 ! 04 4 4.224e+09 3.2e+07 1 3.2e+07 ! 05 5 4.416e+09 3.2e+07 1 3.2e+07 ! 06 6 4.512e+09 3.2e+07 1 3.2e+07 ! 07 7 4.544e+09 3.2e+07 1 3.2e+07 ! 08 8 4.576e+09 3.2e+07 1 3.2e+07 ! ! Polarization(s): RR ! ! Read 94 lines of history. ! ! Reading 15136 visibilities. select rr, 1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16 ! Restricting channel ranges to the available 8 channels. ! Selecting polarization: RR, channels: 1..8 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 ! Reading IF 5 channels: 5..5 ! Reading IF 6 channels: 6..6 ! Reading IF 7 channels: 7..7 ! Reading IF 8 channels: 8..8 print "field_size =", field_size ! field_size = 1024 print "field_cell =", field_cell ! field_cell = 0.3 print "taper_size =", taper_size ! taper_size = 40 ![@/opt64/bin/pima_mupet_02.dfm J2259-3548_C] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.04 float dynam dynam = 6.0 float amp_soltime1 amp_soltime1 = 60 float amp_soltime2 amp_soltime2 = 5 float phase_soltime1 phase_soltime1=10 float phase_soltime2 phase_soltime2=0.5 float phase_soltime phase_soltime=phase_soltime1 float ampcor_selflim ampcor_selflim=1.20 float thresh thresh = 0.1 float win_mult win_mult = 1.8 float time_av time_av = 30 float old_peak float new_peak float flux_cutoff print "===============================================================" ! =============================================================== ! print "=== Difmap script: pima_mupet_02.dvm version of 2017.12.26 === " ! === Difmap script: pima_mupet_02.dvm version of 2017.12.26 === ! mapsize field_size, field_cell ! Map grid = 1024x1024 pixels with 0.300x0.300 milli-arcsec cellsize. phase_soltime=phase_soltime1 print "uvstat(rms)=",uvstat(rms),"Jy" ! uvstat(rms)= 0.0380863 Jy startmod ! Applying default point source starting model. ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! A total of 178 telescope corrections were flagged in sub-array 2. ! A total of 184 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 178 telescope corrections were flagged in sub-array 2. ! A total of 184 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 178 telescope corrections were flagged in sub-array 2. ! A total of 184 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 178 telescope corrections were flagged in sub-array 2. ! A total of 184 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 5. ! A total of 178 telescope corrections were flagged in sub-array 2. ! A total of 184 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 6. ! A total of 178 telescope corrections were flagged in sub-array 2. ! A total of 184 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 7. ! A total of 178 telescope corrections were flagged in sub-array 2. ! A total of 184 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 8. ! A total of 178 telescope corrections were flagged in sub-array 2. ! A total of 184 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.999836Jy sigma=20.642604 ! Fit after self-cal, rms=0.982629Jy sigma=20.590055 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. peakwin win_mult ! Inverting map and beam ! Estimated beam: bmin=1.43 mas, bmaj=10.09 mas, bpa=-10.25 degrees ! Estimated noise=0.845687 mJy/beam. ! Added new window around map position (0, 0.3). flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0161426 Jy ! Component: 100 - total flux cleaned = 0.0164479 Jy ! Total flux subtracted in 100 components = 0.0164479 Jy ! Clean residual min=-0.002837 max=0.002812 Jy/beam ! Clean residual mean=-0.000004 rms=0.000896 Jy/beam ! Combined flux in latest and established models = 0.0164479 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.0164479 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.033482Jy sigma=0.630614 ! Fit after self-cal, rms=0.033466Jy sigma=0.630346 ! Inverting map print "============== Finished uniform weighting CLEAN ==============" ! ============== Finished uniform weighting CLEAN ============== ! uvw 0,-2 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -2. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.965 mas, bmaj=10.97 mas, bpa=-9.147 degrees ! Estimated noise=0.288551 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000486026 Jy ! Component: 100 - total flux cleaned = 0.0005508 Jy ! Component: 150 - total flux cleaned = 0.000591884 Jy ! Component: 200 - total flux cleaned = 0.000626918 Jy ! Total flux subtracted in 200 components = 0.000626918 Jy ! Clean residual min=-0.001108 max=0.001213 Jy/beam ! Clean residual mean=-0.000009 rms=0.000316 Jy/beam ! Combined flux in latest and established models = 0.0170748 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 16 model components to the UV plane model. ! The established model now contains 22 components and 0.0170748 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.033460Jy sigma=0.630095 ! Fit after self-cal, rms=0.033459Jy sigma=0.630077 ! Inverting map print "============== Finished natural weighting CLEAN ==============" ! ============== Finished natural weighting CLEAN ============== ! gscale ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Amplitude normalization factor in sub-array 1: 1.02291 ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 FD 0.77 KP 1.18 LA 0.93 ! MK 0.93 OV 0.96 PT 1.13 ! ! Amplitude normalization factor in sub-array 2: 1 ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* SC 0.00* ! ! Amplitude normalization factor in sub-array 3: 1 ! Telescope amplitude corrections in sub-array 3: ! KP 0.00* OV 0.00* ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 1.0527 ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.92 KP 1.00 LA 0.88 ! MK 0.94 OV 0.96 PT 0.93 ! ! Amplitude normalization factor in sub-array 2: 1 ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* SC 0.00* ! ! Amplitude normalization factor in sub-array 3: 1 ! Telescope amplitude corrections in sub-array 3: ! KP 0.00* OV 0.00* ! ! ! Correcting IF 3. ! Amplitude normalization factor in sub-array 1: 0.992795 ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 FD 0.90 KP 1.19 LA 0.92 ! MK 1.00 OV 1.08 PT 1.01 ! ! Amplitude normalization factor in sub-array 2: 1 ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* SC 0.00* ! ! Amplitude normalization factor in sub-array 3: 1 ! Telescope amplitude corrections in sub-array 3: ! KP 0.00* OV 0.00* ! ! ! Correcting IF 4. ! Amplitude normalization factor in sub-array 1: 0.941931 ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 0.93 KP 1.48 LA 0.93 ! MK 1.02 OV 1.02 PT 1.02 ! ! Amplitude normalization factor in sub-array 2: 1 ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* SC 0.00* ! ! Amplitude normalization factor in sub-array 3: 1 ! Telescope amplitude corrections in sub-array 3: ! KP 0.00* OV 0.00* ! ! ! Correcting IF 5. ! Amplitude normalization factor in sub-array 1: 1.07236 ! Telescope amplitude corrections in sub-array 1: ! BR 0.49 FD 1.00 KP 0.99 LA 0.94 ! MK 0.97 OV 1.11 PT 1.02 ! ! Amplitude normalization factor in sub-array 2: 1 ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* SC 0.00* ! ! Amplitude normalization factor in sub-array 3: 1 ! Telescope amplitude corrections in sub-array 3: ! KP 0.00* OV 0.00* ! ! ! Correcting IF 6. ! Amplitude normalization factor in sub-array 1: 0.928176 ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 FD 1.10 KP 1.17 LA 0.77 ! MK 1.14 OV 1.17 PT 1.14 ! ! Amplitude normalization factor in sub-array 2: 1 ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* SC 0.00* ! ! Amplitude normalization factor in sub-array 3: 1 ! Telescope amplitude corrections in sub-array 3: ! KP 0.00* OV 0.00* ! ! ! Correcting IF 7. ! Amplitude normalization factor in sub-array 1: 0.933916 ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 1.30 KP 1.12 LA 0.93 ! MK 1.06 OV 1.07 PT 1.05 ! ! Amplitude normalization factor in sub-array 2: 1 ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* SC 0.00* ! ! Amplitude normalization factor in sub-array 3: 1 ! Telescope amplitude corrections in sub-array 3: ! KP 0.00* OV 0.00* ! ! ! Correcting IF 8. ! Amplitude normalization factor in sub-array 1: 0.944948 ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 1.07 KP 1.16 LA 0.93 ! MK 1.15 OV 0.98 PT 1.08 ! ! Amplitude normalization factor in sub-array 2: 1 ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* SC 0.00* ! ! Amplitude normalization factor in sub-array 3: 1 ! Telescope amplitude corrections in sub-array 3: ! KP 0.00* OV 0.00* ! ! ! Fit before self-cal, rms=0.033459Jy sigma=0.630077 ! Fit after self-cal, rms=0.032049Jy sigma=0.627722 selfcal false, false, phase_soltime ! Performing phase self-cal over 10 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.032049Jy sigma=0.627722 ! Fit after self-cal, rms=0.032050Jy sigma=0.627700 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.994 mas, bmaj=10.7 mas, bpa=-8.851 degrees ! Estimated noise=0.274712 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.000494708 Jy ! Component: 100 - total flux cleaned = -0.000445964 Jy ! Component: 150 - total flux cleaned = -0.000420734 Jy ! Component: 200 - total flux cleaned = -0.000400427 Jy ! Total flux subtracted in 200 components = -0.000400427 Jy ! Clean residual min=-0.000679 max=0.000810 Jy/beam ! Clean residual mean=0.000015 rms=0.000213 Jy/beam ! Combined flux in latest and established models = 0.0166744 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 28 model components to the UV plane model. ! The established model now contains 46 components and 0.0166744 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.032046Jy sigma=0.627428 ! Fit after self-cal, rms=0.032045Jy sigma=0.627416 ! Inverting map print "============== Finished amplitude gscale SELF-CAL ==============" ! ============== Finished amplitude gscale SELF-CAL ============== ! phase_soltime=phase_soltime2 selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.032045Jy sigma=0.627416 ! Fit after self-cal, rms=0.032016Jy sigma=0.626497 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000129532 Jy ! Component: 100 - total flux cleaned = 0.00014111 Jy ! Component: 150 - total flux cleaned = 0.000151648 Jy ! Component: 200 - total flux cleaned = 0.00016162 Jy ! Total flux subtracted in 200 components = 0.00016162 Jy ! Clean residual min=-0.000662 max=0.000786 Jy/beam ! Clean residual mean=0.000015 rms=0.000208 Jy/beam ! Combined flux in latest and established models = 0.016836 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 14 model components to the UV plane model. ! The established model now contains 51 components and 0.016836 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.032014Jy sigma=0.626464 ! Fit after self-cal, rms=0.032014Jy sigma=0.626406 ! Inverting map print "=== Finished natural weighting clean with shorter phase_soltime " ! === Finished natural weighting clean with shorter phase_soltime ! dynam = dynam - 0.25 restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.994 x 10.7 at -8.851 degrees (North through East) ! Clean map min=-0.00065493 max=0.017867 Jy/beam if(peak(flux) > thresh) selfcal true, true, amp_soltime1 selfcal false, false, phase_soltime flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) print "============== Finished amplitude self-cal ==============" end if print "============== Clearing model and starting over ==========" ! ============== Clearing model and starting over ========== clrmod true,true,true ! clrmod: Cleared the established, tentative and continuum models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter, clean_gain ! Inverting map and beam ! Estimated beam: bmin=1.436 mas, bmaj=9.821 mas, bpa=-10.24 degrees ! Estimated noise=0.816055 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0156251 Jy ! Component: 100 - total flux cleaned = 0.0164985 Jy ! Component: 150 - total flux cleaned = 0.0163226 Jy ! Component: 200 - total flux cleaned = 0.0162734 Jy ! Total flux subtracted in 200 components = 0.0162734 Jy ! Clean residual min=-0.002337 max=0.002345 Jy/beam ! Clean residual mean=0.000003 rms=0.000705 Jy/beam ! Combined flux in latest and established models = 0.0162734 Jy uvw 0,-2 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -2. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 22 model components to the UV plane model. ! The established model now contains 22 components and 0.0162734 Jy ! Inverting map and beam ! Estimated beam: bmin=1.994 mas, bmaj=10.7 mas, bpa=-8.851 degrees ! Estimated noise=0.274712 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000296685 Jy ! Component: 100 - total flux cleaned = 0.00037609 Jy ! Component: 150 - total flux cleaned = 0.000397996 Jy ! Component: 200 - total flux cleaned = 0.000447767 Jy ! Total flux subtracted in 200 components = 0.000447767 Jy ! Clean residual min=-0.000671 max=0.000843 Jy/beam ! Clean residual mean=0.000014 rms=0.000217 Jy/beam ! Combined flux in latest and established models = 0.0167212 Jy ! Adding 15 model components to the UV plane model. ! The established model now contains 36 components and 0.0167212 Jy ! Inverting map clean ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 4.29012e-05 Jy ! Component: 100 - total flux cleaned = 8.00581e-05 Jy ! Component: 150 - total flux cleaned = 0.000111852 Jy ! Component: 200 - total flux cleaned = 0.000130666 Jy ! Total flux subtracted in 200 components = 0.000130666 Jy ! Clean residual min=-0.000685 max=0.000823 Jy/beam ! Clean residual mean=0.000015 rms=0.000211 Jy/beam ! Combined flux in latest and established models = 0.0168519 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 40 components and 0.0168519 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.032017Jy sigma=0.626456 ! Fit after self-cal, rms=0.032016Jy sigma=0.626455 wmodel J2259-3548_C_map.mod ! Writing 40 model components to file: J2259-3548_C_map.mod wobs J2259-3548_C_uvs.fits ! Writing UV FITS file: J2259-3548_C_uvs.fits wwins J2259-3548_C_map.win ! wwins: Wrote 1 windows to J2259-3548_C_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000278446 Jy ! Component: 100 - total flux cleaned = 0.000411606 Jy ! Component: 150 - total flux cleaned = 0.000464582 Jy ! Component: 200 - total flux cleaned = 0.000523244 Jy ! Component: 250 - total flux cleaned = 0.000558381 Jy ! Component: 300 - total flux cleaned = 0.000617177 Jy ! Component: 350 - total flux cleaned = 0.000656912 Jy ! Component: 400 - total flux cleaned = 0.000717376 Jy ! Component: 450 - total flux cleaned = 0.000767575 Jy ! Component: 500 - total flux cleaned = 0.000815641 Jy ! Component: 550 - total flux cleaned = 0.000842186 Jy ! Component: 600 - total flux cleaned = 0.000867169 Jy ! Component: 650 - total flux cleaned = 0.000885318 Jy ! Component: 700 - total flux cleaned = 0.000908853 Jy ! Component: 750 - total flux cleaned = 0.000937354 Jy ! Component: 800 - total flux cleaned = 0.000965113 Jy ! Component: 850 - total flux cleaned = 0.000986639 Jy ! Component: 900 - total flux cleaned = 0.00100242 Jy ! Component: 950 - total flux cleaned = 0.00102805 Jy ! Component: 1000 - total flux cleaned = 0.00105321 Jy ! Component: 1050 - total flux cleaned = 0.00107299 Jy ! Component: 1100 - total flux cleaned = 0.00109728 Jy ! Component: 1150 - total flux cleaned = 0.00111633 Jy ! Component: 1200 - total flux cleaned = 0.00113516 Jy ! Component: 1250 - total flux cleaned = 0.00115367 Jy ! Component: 1300 - total flux cleaned = 0.00115825 Jy ! Component: 1350 - total flux cleaned = 0.00116282 Jy ! Component: 1400 - total flux cleaned = 0.00117176 Jy ! Component: 1450 - total flux cleaned = 0.00117176 Jy ! Component: 1500 - total flux cleaned = 0.00117618 Jy ! Component: 1550 - total flux cleaned = 0.00118933 Jy ! Component: 1600 - total flux cleaned = 0.00119801 Jy ! Component: 1650 - total flux cleaned = 0.00120663 Jy ! Component: 1700 - total flux cleaned = 0.00121095 Jy ! Component: 1750 - total flux cleaned = 0.00122805 Jy ! Component: 1800 - total flux cleaned = 0.00124507 Jy ! Component: 1850 - total flux cleaned = 0.00126203 Jy ! Component: 1900 - total flux cleaned = 0.00128315 Jy ! Component: 1950 - total flux cleaned = 0.00129579 Jy ! Component: 2000 - total flux cleaned = 0.00131683 Jy ! Component: 2050 - total flux cleaned = 0.00133784 Jy ! Component: 2100 - total flux cleaned = 0.00135041 Jy ! Component: 2150 - total flux cleaned = 0.00135042 Jy ! Component: 2200 - total flux cleaned = 0.00136301 Jy ! Component: 2250 - total flux cleaned = 0.00137975 Jy ! Component: 2300 - total flux cleaned = 0.00137976 Jy ! Component: 2350 - total flux cleaned = 0.00137557 Jy ! Component: 2400 - total flux cleaned = 0.00138395 Jy ! Component: 2450 - total flux cleaned = 0.00139656 Jy ! Component: 2500 - total flux cleaned = 0.00140076 Jy ! Component: 2550 - total flux cleaned = 0.00141336 Jy ! Component: 2600 - total flux cleaned = 0.00141334 Jy ! Component: 2650 - total flux cleaned = 0.00142175 Jy ! Component: 2700 - total flux cleaned = 0.00143855 Jy ! Component: 2750 - total flux cleaned = 0.0014554 Jy ! Component: 2800 - total flux cleaned = 0.00146802 Jy ! Component: 2850 - total flux cleaned = 0.00147647 Jy ! Component: 2900 - total flux cleaned = 0.00148913 Jy ! Component: 2950 - total flux cleaned = 0.00151034 Jy ! Component: 3000 - total flux cleaned = 0.0015273 Jy ! Component: 3050 - total flux cleaned = 0.00154436 Jy ! Component: 3100 - total flux cleaned = 0.00156148 Jy ! Component: 3150 - total flux cleaned = 0.00159148 Jy ! Component: 3200 - total flux cleaned = 0.0016259 Jy ! Component: 3250 - total flux cleaned = 0.00165183 Jy ! Component: 3300 - total flux cleaned = 0.00167351 Jy ! Component: 3350 - total flux cleaned = 0.00170399 Jy ! Component: 3400 - total flux cleaned = 0.00174341 Jy ! Component: 3450 - total flux cleaned = 0.00176982 Jy ! Component: 3500 - total flux cleaned = 0.00180074 Jy ! Component: 3550 - total flux cleaned = 0.00184069 Jy ! Component: 3600 - total flux cleaned = 0.00186748 Jy ! Component: 3650 - total flux cleaned = 0.00189885 Jy ! Component: 3700 - total flux cleaned = 0.00193492 Jy ! Component: 3750 - total flux cleaned = 0.00197119 Jy ! Component: 3800 - total flux cleaned = 0.00200771 Jy ! Component: 3850 - total flux cleaned = 0.00203063 Jy ! Component: 3900 - total flux cleaned = 0.00206284 Jy ! Component: 3950 - total flux cleaned = 0.00209982 Jy ! Component: 4000 - total flux cleaned = 0.00213243 Jy ! Component: 4050 - total flux cleaned = 0.00216053 Jy ! Total flux subtracted in 4096 components = 0.00218876 Jy ! Clean residual min=-0.000264 max=0.000284 Jy/beam ! Clean residual mean=0.000004 rms=0.000097 Jy/beam ! Combined flux in latest and established models = 0.0190406 Jy keep ! Adding 243 model components to the UV plane model. ! The established model now contains 283 components and 0.0190406 Jy ![Exited script file: /opt64/bin/pima_mupet_02.dfm] wmap /vlbi/vcs9/uvm//J2259-3548_C_a_map.fits ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.994 x 10.7 at -8.851 degrees (North through East) ! Clean map min=-0.00051057 max=0.018036 Jy/beam ! Writing clean map to FITS file: /vlbi/vcs9/uvm//J2259-3548_C_a_map.fits wmodel /vlbi/vcs9/uvm//J2259-3548_C_a_map.mod ! Writing 283 model components to file: /vlbi/vcs9/uvm//J2259-3548_C_a_map.mod wobs /vlbi/vcs9/uvm//J2259-3548_C_a_uvs.fits ! Writing UV FITS file: /vlbi/vcs9/uvm//J2259-3548_C_a_uvs.fits wwins /vlbi/vcs9/uvm//J2259-3548_C_a_map.win ! wwins: Wrote 2 windows to /vlbi/vcs9/uvm//J2259-3548_C_a_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.0180362 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00010965 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.82383 1.82383 3.64765 7.29531 14.5906 29.1812 58.3625 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0003 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.018 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 164.489 quit ! Quitting program ! Log file /vlbi/vcs9/uvm//J2259-3548_C_a_dfm.log closed on Tue Dec 26 23:13:36 2017